Differential solar rotation - Inhomogeneity rather than anisotropy

Details Differential solar rotation - Inhomogeneity rather than anisotropy Differential solar rotation - Inhomogeneity rather than anisotropy

Jun 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986pazh...12..410k&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 12, May 1986, p. 410-416) Soviet Astronomy Letters (ISSN 0360-0327), vol. 12, May-June

Astronomy and Astrophysics

Astronomy

2

Anisotropy, Inhomogeneity, Solar Rotation, Stellar Models, Angular Velocity, Benard Cells, Density Distribution, Energy Dissipation

Scientific paper

The cyclonic convection cells in a rotating, density-stratified medium
will transport angular momentum efficiently, thereby making the rotation
differential. An approximate theory for the angular momentum flows
yields a relation between the rotational velocity and the coordinates
which is in qualitative accord with the behavior observed on the sun.

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